计算声子谱以及热力学性质的综述

paolo.giannozzi@uniud.it
Eyvaz Isaev
Department of Physics, Chemistry and Biology (IFM) Linköping University Sweden Theoretical Physics Department Moscow State Institute of Steel and Alloys Russia
Reviews in Mineralogy & Geochemistry Vol. 71 pp. XXX-XXX, 2009 Copyright © Mineralogical Society of Amperties of Materials from Ab Initio Quasi-Harmonic Phonons
Thermal properties and the Quasi-Harmonic Approximation
The low-temperature specific heat of solids is experimentally found to vanish as the cube of the temperature, with a cubic coefficient that is system-specific (Kittel 1996; Wallace 1998). This is contrary to the predictions of classical statistical mechanics, according to which the heat capacity of a system of harmonic oscillators does not depend on temperature, nor on its spectrum. One of the landmarks of modern solid-state physics, that greatly contributed to the establishment of our present quantum-mechanical picture of matter, is the Debye model for the heat capacity of solids. This model naturally explains the low-temperature specific heat of solids in terms of the (quantum) statistical mechanics of an ensemble of harmonic oscillators, which can in turn be pictorially described as a gas of non-interacting quasi-particles obeying the Bose-Einstein statistics (phonons). The internal energy of a single harmonic oscillator of angular frequency ω, in thermal equilibrium at temperature T, is:
1529-6466/09/0071-0003$05.00 DOI: 10.2138/rmg.2009.71.3
Baroni_etal.indd 1
12/9/2009 2:15:59 PM
2
Baroni, Giannozzi, Isaev
long simulation times, and by the importance of long-wavelength collective motions (phonons), which would require large simulation cells. Both difficulties are successfully dealt with in the quasi-harmonic approximation (QHA) where the thermal properties of solid materials are traced back to those of a system of non-interacting phonons (whose frequencies are however allowed to depend on volume or on other thermodynamic constraints). An additional advantage of the QHA is that it accounts for quantum-mechanical zero-point effects, which would not be accessible to molecular dynamics with classical nuclear motion. The availability of suitable techniques to calculate the vibrational properties of extended materials using a combination of DFT and linear-response techniques (resulting in the so-called density-functional perturbation theory, DFPT; Baroni et al. 1987, 2001) makes it possible to combine the QHA with DFT. The resulting simulation methodology has shown to be remarkably accurate in a wide temperature range, extending up to not very far from the melting line and has been applied to a wide variety of systems, including many which are relevant to the Earth sciences. This paper gives a short overview of the calculation of thermal properties of materials in the framework of the QHA, using DFT. The paper is organized as follows: in the “Thermal Properties and the QuasiHarmonic Approximation” section, we introduce some of the thermal properties of interest and describe how they can be calculated in the framework of the QHA; in the “Ab Initio Phonons” section, we describe the DFPT approach to lattice dynamics; in the “Computer Codes” section, we briefly introduce some of the computer codes that can be used to perform this task; in the “Applications” section, we review some of the application of the first-principles QHA to the study of the thermal properties of materials; finally, the last section contains our conclusions.
eyvaz_isaev@
Introduction
Computer simulations allow for the investigation of many materials properties and processes that are not easily accessible in the laboratory. This is particularly true in the Earth sciences, where the relevant pressures and temperatures may be so extreme that no experimental techniques can operate at those conditions. Computer modeling is often the only source of information on the properties of materials that, combined with indirect evidence (such as seismic data), allows one to discriminate among competing planetary models. Many computer simulations are performed using effective inter-atomic potentials tailored to reproduce some experimentally observed properties of the materials being investigated. The remoteness of the physically interesting conditions from those achievable in the laboratory, as well as the huge variety of different atomic coordination and local chemical state occurring in the Earth interior, make the dependability of semi-empirical potentials questionable. First-principles techniques based on density-functional theory (DFT) (Hohenberg and Kohn 1964; Kohn and Sham 1965) are much more predictive, not being biased by any prior experimental input, and have demonstrated a considerable accuracy in a wide class of materials and variety of external conditions. The importance of thermal effects in the range of phenomena interesting to the Earth sciences makes a proper account of atomic motion essential. Traditionally, this is achieved using molecular dynamics techniques which have been successfully combined with DFT in the first-principles molecular dynamics technique of Car and Parrinello (1985). Well below the melting temperature, the numerical efficiency of molecular dynamics is limited by the lack of ergodicity, which would require